The best-fitting values of Photon indices from the X-ray afterglow spectral modelling for different temporal segments. We have frozen the host hydrogen column density, obtained from SED 3 (see Section 2.5).
| Time (s) . | |$\rm Photon ~index$| . | Mode . |
|---|---|---|
| 63–65 196 | 1.59 ± 0.09 | WT+PC |
| 63–200 | 1.51 ± 0.03 | WT |
| 200–2200 | 1.61 ± 0.02 | WT |
| 5600–2 × 105 | 1.63 ± 0.09 | PC |
| Time (s) . | |$\rm Photon ~index$| . | Mode . |
|---|---|---|
| 63–65 196 | 1.59 ± 0.09 | WT+PC |
| 63–200 | 1.51 ± 0.03 | WT |
| 200–2200 | 1.61 ± 0.02 | WT |
| 5600–2 × 105 | 1.63 ± 0.09 | PC |
The best-fitting values of Photon indices from the X-ray afterglow spectral modelling for different temporal segments. We have frozen the host hydrogen column density, obtained from SED 3 (see Section 2.5).
| Time (s) . | |$\rm Photon ~index$| . | Mode . |
|---|---|---|
| 63–65 196 | 1.59 ± 0.09 | WT+PC |
| 63–200 | 1.51 ± 0.03 | WT |
| 200–2200 | 1.61 ± 0.02 | WT |
| 5600–2 × 105 | 1.63 ± 0.09 | PC |
| Time (s) . | |$\rm Photon ~index$| . | Mode . |
|---|---|---|
| 63–65 196 | 1.59 ± 0.09 | WT+PC |
| 63–200 | 1.51 ± 0.03 | WT |
| 200–2200 | 1.61 ± 0.02 | WT |
| 5600–2 × 105 | 1.63 ± 0.09 | PC |
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.
